Stereo Pairs 
An explanation of stereo pairs and their use (PDF)  

Planned stereo pairs have suitable stereo convergence angles and illumination by design. In addition to planned stereo pairs, the Pairendipity software can identify overlapping HiRISE images that are serendipitously suitable for stereo processing and find stereo pairs within the CTX dataset.

Planned HiRISE stereo pairs are listed in the “Stereo Pair List (CSV)” link below. Since this list is based on produced stereo anaglyphs it also contains a few serendipitous pairs that underwent special processing. Most serendipitous HiRISE stereo pairs are listed in the “Pairendipity Stereo” link, while CTX stereo pairs are listed in “Pairendipity CTX Stereo”.

Images taken close together in time minimize illumination and frost differences and are especially useful (see the Delta-Days column in the Pairendipity files or difference the orbit numbers in the image IDs in the Stereo Pair List file). Stereo pairs with both images planned within the same 14-day (168-orbit) operations cycle are known as SPORCs.

Crater Floor Outcrop:   ESP_067980_2160   ESP_063970_2160   (Interval in Earth days: 312)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
35.60

0.43

-22.

-12.2

54.5

59.7

Cross-Cutting Faults Southeast of Melas Chasma:   ESP_067732_1650   ESP_073746_1650   (Interval in Earth days: 468)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.9

290.

-14.

16.69

41.5

54.0

Inverted Channel in Cusus Valles:   ESP_067833_1960   ESP_067965_1960   (Interval in Earth days: 11)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
16.05

49.8

5.88

-3.77

43.8

44.2

Valleys in Crater Northeast of Argyre Region:   ESP_067704_1500   ESP_073784_1500   (Interval in Earth days: 474)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-29.6

334.

7.13

20.86

44.0

53.7

Channels in Orson Welles Crater:   ESP_067797_1790   ESP_075433_1790   (Interval in Earth days: 595)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.14

314.

4.35

-15.7

39.8

44.2

Floor of Lampland Crater:   ESP_068036_1440   ESP_073430_1440   (Interval in Earth days: 421)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-35.6

280.

-4.6

13.35

52.9

59.9

Mounds in Acidalia Planitia:   ESP_068074_2280   ESP_068483_2280   (Interval in Earth days: 32)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
47.47

312.

-7.6

26.38

59.5

53.0

Collapse Terrain near Orson Welles Crater:   ESP_068061_1785   ESP_072677_1785   (Interval in Earth days: 360)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-1.50

313.

1.23

21.77

41.5

55.4

Terrain Sample:   ESP_067995_1650   ESP_067520_1650   (Interval in Earth days: 37)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
-14.7

313.

24.1

7.839

41.1

38.2

Features in Echus Chasma:   ESP_068049_1805   ESP_072665_1805   (Interval in Earth days: 360)
Center lat.Center long.1st half roll angle2nd half roll angle1st half incidence angle2nd half incidence angle
0.707

279.

4.52

27.80

41.1

54.4


  


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